A higher dimensional stationary rotating black hole must be axisymmetric
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Publication:2385029
DOI10.1007/s00220-007-0216-4zbMath1128.83028arXivgr-qc/0605106OpenAlexW2022227375WikidataQ125975074 ScholiaQ125975074MaRDI QIDQ2385029
Stefan Hollands, Robert M. Wald, Akihiro Ishibashi
Publication date: 11 October 2007
Published in: Communications in Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0605106
Black holes (83C57) Applications of global differential geometry to the sciences (53C80) Kaluza-Klein and other higher-dimensional theories (83E15)
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